Калашёв Олег Евгеньевич Группа Т ПРНД=121,96
Калашев Олег Евгеньевич
дата рожд. 4 янв 1976, кандидат физ-мат наук, старший научный
сотрудник, отдел теоретической физики
Расчет ПРНД за 2011-2012гг:
Статьи в реферируемых зарубежных журналах:
Role of line-of-sight cosmic ray interactions in forming the spectra of
distant blazars in TeV gamma rays and high-energy neutrinos.
Warren Essey, (UCLA) , Oleg Kalashev, (Moscow, INR) , Alexander Kusenko,
(UCLA & Tokyo U., IPMU) , John F. Beacom, (Ohio State U.) . Nov 2010. 18pp.
Published in Astrophys.J.731:51,2011.
ПРНД=6.063*30/4=45.47
Secondary photons and neutrinos from cosmic rays produced by distant blazars
Warren Essey, Oleg E. Kalashev, Alexander Kusenko, John F. Beacom
Phys.Rev.Lett.104:141102,2010
ПРНД=7.328*30/4=54.96
Препринты:
Gamma-Ray Constraints on Maximum Cosmogenic Neutrino Fluxes and UHECR
Source Evolution Models.
Graciela B. Gelmini, Oleg Kalashev, Dmitri V. Semikoz
e-Print: arXiv:1107.1672 [astro-ph.CO]
ПРНД=4/3=1.33
Role of line-of-sight cosmic ray interactions in forming the spectra of
distant blazars in TeV gamma rays and high-energy neutrinos
Warren Essey, Oleg Kalashev, Alexander Kusenko, John F. Beacom
e-Print: arXiv:1011.6340 [astro-ph.HE]
ПРНД=4/4=1
Доклады на конференциях:
Secondary neutrinos and multi-TeV photons from distant blazars
Quarks 2010 International Conference, Kolomna
ПРНД=6
Restricting cosmogenic neutrino fluxes with Fermi 3 years data,
Nusky 2011 International Workshopn on Cosmic Rays and Cosmic Neutrinos,
20-25 June 2011 Trieste Italy
ПРНД=6
Restrictions on cosmogenic neutrinos and UHECR from Fermi 3 years data
12th International Conference on Topics in Astroparticle and Underground
Physics
5–9 September 2011, Munich, Germany
ПРНД=6
Search for global asymmetry of UHECR arrival directions with
space-based detectors (TUS, JEM-EUSO)
Pavel Klimov, Oleg Kalashev, Boris Khrenov, Sergey Sharakin and Sergey
Troitsky
31st International Cosmic Ray Conference, Lodz, Polland, July 2009
ПРНД=6 / 5 = 1.2
Итого суммарный
ПРНД=45.47+54.96+1.33+1+6+6+6+1.2=121.96